scholarly journals ELECTROSTATIC ION THRUSTERS - TOWARDS PREDICTIVE MODELING

2015 ◽  
Vol 55 (1) ◽  
pp. 7-13
Author(s):  
Julia Duras ◽  
Oleksander Kalentev ◽  
Ralf Schneider ◽  
Konstantin Matyash ◽  
Karl Felix Lüskow ◽  
...  

For satellite missions, thrusters have to be qualified in large vacuum vessels to simulate space environment. One caveat of these experiments is the possible  modification of the beam properties due to the interaction of the energetic ions with the  vessel walls. Impinging ions can produce sputtered impurities or secondary  electrons from the wall. These can stream back into the acceleration channel of the  thruster and produce co-deposited layers. Over the long operation time of thousands  of hours, such layers can modify the optimized geometry and induce changes of the ion beam properties, e.g. broadening of the angular distribution and thrust reduction. To study such effects, a Monte Carlo code for the simulation of the interaction of ion thruster beams with vessel  walls was developed. Strategies to overcome sputter limitations by additional baffles are  studied with the help of this Monte-Carlo erosion code.<br /><br />

2018 ◽  
Vol 122 (1255) ◽  
pp. 1425-1441 ◽  
Author(s):  
C. Lu ◽  
P. Qiu ◽  
Y. Cao ◽  
T.P. Zhang ◽  
J.J. Chen

ABSTRACTCharge Exchange (CEX) ion is the main factor causing the plume pollution. The distribution of CEX ions is determined by the distribution of beam ions and neutral atoms. Hence, the primary problem in the study of the plume is how to accurately simulate the distribution of beam ions and neutral atoms. At present, the most commonly used model utilised for the plume simulation is the analytical model proposed by Roy for the plume simulation of the NASA Solar Technology Application Readiness (NSTAR) ion thruster. However, this analytical model can only be applied to the ion beam with small divergence angles. In addition, the analytical model is no longer applicable to the simulation for the plume of a new type of ion thruster that appeared recently, which is called the annular ion thruster. In this paper, a 3D particle model is proposed for the plume simulation of ion thrusters consisting of the particle model for beam ions, the Direct Simulation Monte Carlo (DSMC) model for neutral atoms and the Immersed Finite Element-Particle In Cell-Monte Carlo Collision (IFE-PIC-MCC) model for CEX ions. Then, the plume of the NSTAR ion thruster is simulated by both Roy's model and the 3D particle model. The simulation results of both models are then compared with the experimental results. It is shown that the numerical results of the 3D particle model agree well with those of the analytical model and the experimental data. And this 3D particle model can also be used for other electric thrusters.


2004 ◽  
Vol 49 (10) ◽  
pp. 1933-1958 ◽  
Author(s):  
Irena Gudowska ◽  
Nikolai Sobolevsky ◽  
Pedro Andreo ◽  
D evad Belki ◽  
Anders Brahme

2014 ◽  
Vol 41 (6Part16) ◽  
pp. 298-298 ◽  
Author(s):  
I Rinaldi ◽  

2020 ◽  
Vol 91 (1) ◽  
pp. 10901 ◽  
Author(s):  
Patrick Dietz ◽  
Felix Becker ◽  
Konstantin Keil ◽  
Kristof Holste ◽  
Peter J. Klar

Neutralization of the extracted ion beam is a mandatory task for any ion thruster based space mission. The required lifetimes are in the order of ten thousand hours. This requirement is fulfilled by hollow cathodes operating with xenon, but has not been demonstrated for operation with iodine yet. Furthermore, the power consumption as well as the demand on mass flow should be kept as low as possible. Since the halogen iodine seems to be a viable alternative to xenon for operating ion thrusters, a suitable neutralizer concept that can operate with the corrosive gas for the time periods stated above is required. We propose to use a neutralizer based on an inductively coupled rf discharge as alternative to hollow cathodes. We studied the performance of a prototypical neutralizer operating with iodine as well as the inert gases xenon and krypton and compared the experimental studies with the results of global modeling.


2017 ◽  
Vol 62 (18) ◽  
pp. 7482-7504 ◽  
Author(s):  
A Schiavi ◽  
M Senzacqua ◽  
S Pioli ◽  
A Mairani ◽  
G Magro ◽  
...  

2017 ◽  
Vol 62 (16) ◽  
pp. 6784-6803 ◽  
Author(s):  
T Tessonnier ◽  
A Mairani ◽  
S Brons ◽  
P Sala ◽  
F Cerutti ◽  
...  

1981 ◽  
Vol 55 (1-2) ◽  
pp. 119-129 ◽  
Author(s):  
M. L. Roush ◽  
T. D. Andreadis ◽  
O. F. Goktepe

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